Hydrothermal systems associated with martian impact craters

By J. Rathbun, S. Squyres. 2002

160 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/0824448771b000da70385456dc2cd16f56d89963

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In Astronomy and Astrophysics

Citations in the corpus

The timing of martian valley network activity : Constraints from buffered crater counting (2008, background): “Occurrence in association with impact craters is easily understood in terms of the direct heating associated with impact events and the local melting of permafrost or ground ice and snow deposits (Rathbun and Squyres, 2002) to produce valley networks.”
Impact-generated hydrothermal systems capable of forming phyllosilicates on Noachian Mars (2009, background): “Each of these systems was heated by shocked rocks, including any impact melt, and crustal rocks that were uplifted in central peaks and peak rings (Rathbun and Squyres, 2002; Abramov and Kring, 2005, 2007).”
Impact-generated hydrothermal systems on Earth and Mars (2013, background): “These observations are particularly important with respect to Mars, where the focus of impact-generated hydrothermal models has exclusively focused on crater interiors (e.g., Rathbun and Squyres, 2002; Abramov and Kring, 2005; Schwenzer and Kring, 2009).”
Exploration of hydrothermal targets on Mars (2007, methodology): “Hydrothermal modeling conducted by Rathbun and Squyres (2002) AC CE PT ED M AN US CR IP T indicated that a lake could form in a large complex impact crater from the associated heat of the impact, even under current martian atmospheric conditions.”
Impact‐induced hydrothermal activity on early Mars (2005, methodology): “This work presents several specific improvements on Rathbun and Squyres [2002] .”